activity
20152022
most citedObservations of a Magellanic Corona

43 citations · 74 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.GA202243 cited

Observations of a Magellanic Corona

Dhanesh Krishnarao, Andrew J. Fox, Elena D'Onghia +6

The Large and Small Magellanic Clouds (LMC/SMC) are the closest major satellite galaxies of the Milky Way. They are likely on their first passage on an infalling orbit towards our…

astro-ph.GA202015 cited

Evidence for a Rotational Component in the Circumgalactic Medium of Nearby Galaxies

David M. French, Bart P. Wakker

We present results of a study comparing the relative velocity of absorbers to the rotation velocity of nearby galaxy disks in the local universe (). We have…

astro-ph.GA2019

Completing the Hydrogen Census in the Circumgalactic Medium at z~0

D. J. Pisano, A. Fox, D. French +4

Over the past decade, Lyman-alpha and metal line absorption observations have established the ubiquity of a gas-rich circumgalactic medium (CGM) around star-forming galaxies at z~0…

astro-ph.GA20196 cited

Understanding the circumgalactic medium is critical for understanding galaxy evolution

Molly S. Peeples, Peter Behroozi, Rongmon Bordoloi +69

Galaxies evolve under the influence of gas flows between their interstellar medium and their surrounding gaseous halos known as the circumgalactic medium (CGM). The CGM is a major…

astro-ph.GA20178 cited

Probing Large Galaxy Halos at with Automated -Absorption Matching

David M. French, Bart P. Wakker

We present initial results from an ongoing large-scale study of the circumgalactic medium in the nearby Universe ( km/s), using archival Cosmic Origins Spectrograph…

astro-ph.CO20152 cited

Nearby galaxy filaments and the Lya forest: confronting simulations and the UV background with observations

Bart P. Wakker, Audra K. Hernandez, David French +3

Simulations of the formation of large-scale structure predict that dark matter, low density highly ionized gas, and galaxies form 10 40 Mpc scale filaments. These structure are eas…